Astronomers do it Again: Find Organic Molecules Around Gas Planet (w/ Video)
October 20, 2009 by Mary Beth Murrill
The basic chemistry for life has been detected in a second hot gas planet, HD 209458b, depicted in this artist's concept.
(PhysOrg.com) -- Peering far beyond our solar system, NASA researchers have detected the basic chemistry for life in a second hot gas planet, advancing astronomers toward the goal of being able to characterize planets where life could exist. The planet is not habitable but it has the same chemistry that, if found around a rocky planet in the future, could indicate the presence of life.
"It's the second planet outside our solar system in which water, methane and carbon dioxide have been found, which are potentially important for biological processes in habitable planets," said researcher Mark Swain of NASA's Jet Propulsion Laboratory, Pasadena, Calif. "Detecting organic compounds in two exoplanets now raises the possibility that it will become commonplace to find planets with molecules that may be tied to life."
Swain and his co-investigators used data from two of NASA's orbiting Great Observatories, the Hubble Space Telescope and Spitzer Space Telescope, to study HD 209458b, a hot, gaseous giant planet bigger than Jupiter that orbits a sun-like star about 150 light years away in the constellation Pegasus. The new finding follows their breakthrough discovery in December 2008 of carbon dioxide around another hot, Jupiter-size planet, HD 189733b. Earlier Hubble and Spitzer observations of that planet had also revealed water vapor and methane.
This video is not supported by your browser at this time.
The detections were made through spectroscopy, which splits light into its components to reveal the distinctive spectral signatures of different chemicals. Data from Hubble's near-infrared camera and multi-object spectrometer revealed the presence of the molecules, and data from Spitzer's photometer and infrared spectrometer measured their amounts."This demonstrates that we can detect the molecules that matter for life processes," said Swain. Astronomers can now begin comparing the two planetary atmospheres for differences and similarities. For example, the relative amounts of water and carbon dioxide in the two planets is similar, but HD 209458b shows a greater abundance of methane than HD 189733b. "The high methane abundance is telling us something," said Swain. "It could mean there was something special about the formation of this planet."
Other large, hot Jupiter-type planets can be characterized and compared using existing instruments, Swain said. This work will lay the groundwork for the type of analysis astronomers eventually will need to perform in shortlisting any promising rocky Earth-like planets where the signatures of organic chemicals might indicate the presence of life.
Rocky worlds are expected to be found by NASA's Kepler mission, which launched earlier this year, but astronomers believe we are a decade or so away from being able to detect any chemical signs of life on such a body.
If and when such Earth-like planets are found in the future, "the detection of organic compounds will not necessarily mean there's life on a planet, because there are other ways to generate such molecules," Swain said. "If we detect organic chemicals on a rocky, Earth-like planet, we will want to understand enough about the planet to rule out non-life processes that could have led to those chemicals being there."
"These objects are too far away to send probes to, so the only way we're ever going to learn anything about them is to point telescopes at them. Spectroscopy provides a powerful tool to determine their chemistry and dynamics."
More information:
You can follow the history of planet hunting from science fiction to science fact with NASA's PlanetQuest Historic Timeline at http://planetquest … ov/timeline/ .
More information about exoplanets and NASA's planet-finding program is at http://planetquest … jpl.nasa.gov .
-
Hubble Finds Carbon Dioxide on an Extrasolar Planet
Dec 09, 2008 |
not rated yet |
0
-
Hubble Finds First Organic Molecule on an Exoplanet
Mar 19, 2008 |
not rated yet |
0
-
Absence of Water in Distant Planet's Atmosphere Surprises Astronomers
Feb 21, 2007 |
not rated yet |
0
-
Earth-like planets may be found soon
Mar 24, 2008 |
not rated yet |
0
-
Search for the water of life -- Astronomers find water on extra-solar planet
Jul 11, 2007 |
not rated yet |
0
-
Engineers build first sub-10-nm carbon nanotube transistor
Feb 01, 2012 |
4.9 / 5 (30) |
30
-
Something old, something new: Evolution and the structural divergence of duplicate genes
Jan 31, 2012 |
4.6 / 5 (7) |
1
-
The hidden nanoworld of ice crystals: Revealing the dynamic behavior of quasi-liquid layers
Jan 30, 2012 |
5 / 5 (3) |
1
-
Stock market network reveals investor clustering
Jan 27, 2012 |
3.9 / 5 (23) |
8
-
Of microchemistry and molecules: Electronic microfluidic device synthesizes biocompatible probes
Jan 26, 2012 |
5 / 5 (1) |
0
-
Titan's lack of impact craters
22 hours ago
-
Real pictures of black hole eating a star?
Feb 08, 2012
-
Hypothetical way to travel faster than light, but not technically exceed lightspeed
Feb 06, 2012
-
How do scientists monitor the Sun's activity?
Feb 05, 2012
-
Search patterns in observational studies
Feb 05, 2012
-
Derivation of Pogson's law
Feb 03, 2012
- More from Physics Forums - General Astronomy
More news stories
Clam fields found at deep, low-temperature Mariana vents
(PhysOrg.com) -- Scientists have marveled at the unusual life forms thriving at high temperature hydrothermal vents of the deep ocean.
Space & Earth / Earth Sciences
48 minutes ago |
not rated yet |
0
|
Could Venus be shifting gear?
(PhysOrg.com) -- ESAs Venus Express spacecraft has discovered that our cloud-covered neighbour spins a little slower than previously measured. Peering through the dense atmosphere in the infrared, the ...
Space & Earth / Space Exploration
16 minutes ago |
5 / 5 (1) |
0
|
Streams need trees to withstand climate change
(PhysOrg.com) -- More than twenty years of biological monitoring have confirmed the importance of vegetation for protecting Australia's freshwater streams and rivers against the ravages of drought and climate ...
57 minutes ago |
not rated yet |
0
The turbulent birth of super star clusters in galaxy mergers
By combining two of the most advanced telescopes in the world -- the new Atacama Large Millimeter Array (ALMA) and the Very Large Telescope (VLT) of ESO -- a team of French astronomers from the Institut d'astrophysique ...
39 minutes ago |
not rated yet |
0
What does a nebula sound like?
What do things sound like out in the cosmos? Of course, sound waves cant travel through the vacuum of space; however, electromagnetic waves can. These electromagnetic waves can be recorded by devices called spectrographs ...
Space & Earth / Space Exploration
23 minutes ago |
5 / 5 (1) |
0
Seeing colors in music, tasting flavors in shapes may happen in life's early months
Famed violinist Itzhak Perlman sees a deep forest green whenever he plays a B-flat on his Stradivarius' G string. The A on the E string is red.
Is that sleepiness during pregnancy normal or a sign of sleep apnea?
(Medical Xpress) -- Most pregnant women complain of being tired. Some of them however, could be suffering more than normal fatigue associated with their pregnancy; they may have developed obstructive sleep apnea (OSA), a ...
Engineering images bring life to submerged city
(PhysOrg.com) -- Photo-realistic 3D mapping and digital reconstruction of an ancient underwater city in Greece have earned a team from the University of Sydney's Faculty of Engineering and Information Technologies ...
Numeracy: The educational gift that keeps on giving?
(Medical Xpress) -- Cancer risks. Investment alternatives. Calories. Numbers are everywhere in daily life, and they figure into all sorts of decisions. A new article published in Current Directions in Psychological Science, a journal of the Association for Psychological Science, examin ...
New power source discovered
(PhysOrg.com) -- Researchers at the Massachusetts Institute of Technology (MIT) and RMIT University have made a breakthrough in energy storage and power generation.
Measurements from high-energy collisions lead to better understanding of why meson particles disappear
For several years, physicists at the Relativistic Heavy Ion Collider (RHIC) at Brookhaven National Laboratory (BNL), USA, have studied an unusual state of matter called the quarkgluon plasma, which they ...
Oct 20, 2009
Rank: not rated yet
Oct 20, 2009
Rank: not rated yet
Oct 21, 2009
Rank: not rated yet
What are they going to do, come take our jobs? :)
Oct 21, 2009
Rank: 1 / 5 (1)
Both of these essential elements of life exist in the outer layers of stars and in planets that form from the outer layers of supernovae.
Earth, ordinary meteorites and other rocky planets are made primarily of elements from the deep interior of supernovae - Fe, O, Ni, Si, S, Mg and Ca.
Compare a cross section of the onion-skin model of a pre-supernova star with that of the solar system.
With kind regards,
Oliver K. Manuel
Oct 21, 2009
Rank: 1 / 5 (1)
Oct 21, 2009
Rank: 3 / 5 (1)
With kind regards,
Oliver K. Manuel
Oct 22, 2009
Rank: 1 / 5 (1)
If you want to know more about element #10, Neon, google "The Neon Alphabet Game." There you will learn that the dozen different types of Neon alphabetically labeled as Ne-A, Be-B, Ne-C, Ne-D, Ne-E, etc are all products of simple mass fractionation in the Sun.
With kind regards,
Oliver K. Manuel
Oct 22, 2009
Rank: 3 / 5 (2)
Yes, that was my point, and it went right over your head. If neon was in one of the innermost layers of the supernova explosion, the layers you claim formed the terrestrial planets, then where is all the neon? Its absence suggests that there was another force at work in addition to or instead of your supernova hypothesis. This other mechanism is obviously the temperature and phase dependent sorting of elements and chemical compounds that occurs in a system with an energetic central heat source and a cold periphery, such as a protoplanetary disk surrounding a protostar. Your supernova hypothesis is neither necessary nor sufficient to explain the current structure of the solar system.
It's funny that you mention mass fractionation of neon, as that is actually part of the temperature and phase dependent sorting I mentioned.